International FAIR

Boris Sharkov FAIR / MEPhI

Scientific Managing Director, Lomonosov MSU 2015

SwedenFrance IndiaFinland Germany Poland UK Romania Russia Slovenia

UNILAC

SIS18 SIS100/300p-Linac

HESR

CR &RESR

NESR

Cryring

Rare-IsotopeProduction Target

Anti-ProtonProduction Target

100 m

Facility for Antiproton and Ion Research

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FAIR – new international research laboratory to explore the nature and evolution of matter in the Universe

The FAIR Project

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UNILAC

SIS18 SIS100/300p-Linac

HESR

CR &RESR

NESR

Cryring

Rare-IsotopeProduction Target

Anti-ProtonProduction Target

100 m

Facility for Antiproton and Ion Research

Primary Beams

• 1012/s; 1.5 GeV/u; 238U28+

• 1010/s 238U73+ up to 35 GeV/u• 3x1013/s 30 GeV protons

Secondary Beams

Storage and Cooler Rings

• radioactive beams

• 1011 antiprotons 1.5 - 15 GeV/c,

stored and cooledTechnical Challenges • cooled beams, rapid cycling superconducting magnets

• range of radioactive beams up to 1.5 - 2 GeV/u; up to factor 10 000 higher in intensity than presently • antiprotons 3 - 30 GeV

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Facility for Antiproton & Ion Research

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Dense Bulk Plasmas (Ion-beam bunch compression& petawatt-laser)

Dense Bulk Plasmas (Ion-beam bunch compression& petawatt-laser)

Materials Science & Radiation Biology (Ion & antiproton beams)Materials Science & Radiation Biology (Ion & antiproton beams) Accelerator PhysicsAccelerator Physics

UNILAC

SIS18 SIS100/300p-Linac

HESR

CR &RESR

NESR

Cryring

Rare-IsotopeProduction Target

Anti-ProtonProduction Target

100 m

QCD-Phase Diagram(HI beams 2 to 45 GeV/u)QCD-Phase Diagram(HI beams 2 to 45 GeV/u)

Hadron Physics (Stored and cooled14 GeV/c anti-protons)

Hadron Physics (Stored and cooled14 GeV/c anti-protons)

Nuclear Structure & Astrophysics(Rare-isotope beams)Nuclear Structure & Astrophysics(Rare-isotope beams)

Fundamental Symmetries& Ultra-High EM Fields(Antiprotons & highly stripped ions)

Fundamental Symmetries& Ultra-High EM Fields(Antiprotons & highly stripped ions)

• Steering company

• International Convention

• Partners

FAIR GmbH

SwedenFrance IndiaFinland Germany Poland UK Romania Russia Slovenia

Wiesbaden, 2010

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The 4 Scientific Pillars of FAIRAPPA: Atomic, Plasma Physics and Applications

CBM: Compressed Baryonic MatterNUSTAR: Nuclear Structure, Astrophysics and ReactionsPANDA: Antiproton Annihilations at Darmstadt

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The FAIR Project

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NUSTARradioactive ion beams

NUSTARradioactive ion beams

PANDAantiproton beams

PANDAantiproton beams

CBMrelativistic

nuclear collisions

CBMrelativistic

nuclear collisions

APPAions, antiprotons

APPAions, antiprotons

Collaboration Members by Country

9In total: 2500 – 3000 Users from about 50 countries

APPA

• Atomic, Plasma Physics and Applications About 700 members Wide field of science

• basic research to material, biological and medical applications

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APPA

Atomic PhysicsSPARC: 284 members from 26 countriesFLAIR: 144 members from 15 countries

Plasma PhysicsHEDgeHOB & WDM: 175 members from 16 countries

Materials Research and BiophysicsBIOMAT: 110 members from 12 countries

APPA Science Case

• Highest Charge States Extreme Static Fields• Relativistic Energies Extreme Dynamical Fields and Ultrashort

Pulses• High Intensities Very High Energy Densities and Pressures • High Charge at Low Velocity Large Energy Deposition• Low-Energy Anti-Protons Antimatter Research

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planetary interiors

... states of matter common in

astrophysical objects

extreme conditions

... radiation hardness and modification of

materials

Plasma Bio

aerospace engineering

... radiation shielding of cosmic

radiation

Materials

anti-matter

... matter / anti-matter

asymmetry

strong field research

... probing of fundamental laws

of physics

Atomic Physics

SPARC FLAIR HEDgeHOB/WDM MAT/BIOMAT BIO/BIOMAT

NUSTAR

• Nuclear Structure, Astrophysics and Reactions About 800 members

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NUSTAR

Super-FRS

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NUSTAR – Physics Case

Nuclear structure

• Underlying QCD structure → complex nucleon-nucleon force

• Study of exotic short lived nuclei far off stability(proton/ neutron skins or halos, new magic numbers...)

→ Pave way for theoretical framework with predictive power for nuclei beyond experimental reach

Astrophysics

• Origin of the heavy elements?

• Physics of stellar explosions (core-collapse, thermonuclear supernovae, nucleosynthesis)

• Compact objects and the explosions on their surfaces (x-ray bursts)

PANDA

• Antiproton Annihilations at Darmstadt About 500 members

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PANDA

Uniqueness of anti-p probe(no other anti-p facility in this energy range in the world)

PANDA Physics Case

• Gluonic excitations Hybrids, glueballs

• Charmonium states Precision spectroscopy

• Time-like Form factors, nucleon structure

• In medium mass modifications Extension to the charm sector

• Extension of nuclear chart Double hypernuclei

• And much more...

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Direct resonant formation of states with all non-exotic quantum numbers.⟹ excellent precision in mass and width measurement

Comparison with Other Techniques

• e+e- –direct formation limited to J(PC) = 1(- -) –limited resolution for masses and widths for non vector states –sub-MeV widths very difficult or impossible –high L not accessible

• high-energy (several TeV) hadroproduction – high combinatorial background makes discovery of new states very difficult – width measurements limited by detector resolution• B decays (both for e+e- and hadroproduction) – limited J(PC) – C cannot be determined since not conserved in weak decay

Inti Lehmann FAIR, 95th ECFA, 25/7/2014 17

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PANDA Experimental Set-Up

• Fixed target magnetic spectrometer experiment

BeamBeam

Interactionpoint

Interactionpoint

Target SpectrometerTarget Spectrometer Forward SpectrometerForward Spectrometer

SolenoidSolenoid

DipoleDipole

CBM

• Compressed Baryonic Matter About 400 members

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CBM

CBM Physics Case

• The equation-of-state at high baryonic density

• New phases of strongly-interacting matter

• Deconfinement phase transition at high baryonic density

• QCD critical endpoint • Onset of chiral

symmetry restoration at high baryonic density

• Strange matter20

Courtesy of T. Hatsuda

FAIR

RHIC, LHC

2019

2022

20??

2017

Fixed target:L-limited bydetectors

Colliders:scale of L,

in cm-2s-1

SIS-18 (GSI)

Nuclotron-M (JINR)

SPS (NA-49/61, CERN)

AGS (BNL)

RHIC (BNL)

Booster (JINR)

NICA (JINR)

SIS-100 (FAIR)

SIS-300 (FAIR)

2 4 6 8 20 40 60 80

for Au+Au1 10 102

√SNN, GeV

1027

1025

1023

Existing and future HI acceleratorsExisting and future HI accelerators

23CBM – NICA co-operation agreementCBM – NICA co-operation agreementCBM – NICA co-operation agreementCBM – NICA co-operation agreement

Dipolmagnet

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

Electro-magneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Inti Lehmann 25FAIR, 95th ECFA, 25/7/2014

CBM Detector

Modularised Start Version (MSV)

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APPA

CBM/HADESCBM/HADES

NUSTAR

PANDAPANDAModulesM0: SIS100M1: APPAM1: CBM/HADESM2: NUSTARM3: PANDA, NuSTAR,

APPA

M0

M1

M2M3

M3

Cost about 1.6 billion by 2018(1 billion 2005 Euros)

Funding Modules 0-3

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• All numbers in 2005 €escalation until 2018 ca.

+50%i.e. about € 1.6 billion

• Most contributions in-kind

• Discussions with Spain and Italy on-going

• Interested parties• ESA, Saudi Arabia,

Netherlands, China, Turkey, Brazil, Ukraine, S Korea, Japan, USA

B. Sharkov 28

Google Earth for FAIR 7.12.2013

2.5 km

Civil Construction: Satellite’s View

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Type Mass (t)

  5.835.000

Soil out 1.154.000 m3 2.077.200

Soil in 1.078.000 m3 1.940.400

Concrete 519.000 m3 1.283.400

Reinforcement steel 34.000 t 34.000

Other 500.000 t 500.000

Accelerator’s Status

• Progressing well

• SIS 100 dipoles First series del.+tested

• SIS 100 sextopoles Dubna prototype

• HEBT magnets Efremov, St Petersburg

• SIS 100 quadrupoles JINR, Dubna

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ConclusionsConclusions

o Despite of certain delay FAIR is progressing well.

o Rich scientific program and discovery potential already at MSV with beams from SIS100.

o FAIR will explore "unknown territory" of the QCD phase diagram with unprecedented precision.

o Versatile detector configurations for optimal performance are under construction.

o Day-one physics with start version for high interaction rates in preparation.

o Strong an experienced international collaborations are active, more scientists expected to join in the coming years.

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FAIR Science Sketch

QCD phase transition - CBM

temperature

time

Hadron structure - PANDA

Astrophysics andnuclear structure

- NUSTAR

Atomic, applied and plasma physics - APPA

big bang

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Thank you for attention !

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